[HTML][HTML] 25 years of self-organized criticality: solar and astrophysics
MJ Aschwanden, NB Crosby, M Dimitropoulou… - Space Science …, 2016 - Springer
Shortly after the seminal paper “Self-Organized Criticality: An explanation of 1/f noise” by
Bak et al.(1987), the idea has been applied to solar physics, in “Avalanches and the …
Bak et al.(1987), the idea has been applied to solar physics, in “Avalanches and the …
Avalanche models for solar flares (Invited Review)
P Charbonneau, SW McIntosh, HL Liu, TJ Bogdan - Solar Physics, 2001 - Springer
This paper is a pedagogical introduction to avalanche models of solar flares, including a
comprehensive review of recent modeling efforts and directions. This class of flare model is …
comprehensive review of recent modeling efforts and directions. This class of flare model is …
von Kármán–Howarth equation for magnetohydrodynamics and its consequences on third-order longitudinal structure and correlation functions
H Politano, A Pouquet - Physical Review E, 1998 - APS
A derivation in variable dimension of the scaling laws for mixed third-order longitudinal
structure and correlation functions for incompressible magnetized flows is given for arbitrary …
structure and correlation functions for incompressible magnetized flows is given for arbitrary …
The heating of the solar corona
RW Walsh, J Ireland - The Astronomy and Astrophysics Review, 2003 - Springer
The heating of the solar corona has been a fundamental astrophysical issue for over sixty
years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO …
years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO …
[PDF][PDF] Self-organized criticality systems
MJ Aschwanden - Open Aca, 2013 - ulrich-von-kusserow.de
The following chapter provides an overview of the techniques used to understand Self-
Organised Criticality (SOC) by performing computer simulations. Those are of particular …
Organised Criticality (SOC) by performing computer simulations. Those are of particular …
A decade of solar type III radio bursts observed by the Nançay radioheliograph 1998–2008
P Saint-Hilaire, N Vilmer, A Kerdraon - The Astrophysical Journal, 2012 - iopscience.iop.org
We present a statistical survey of almost 10,000 radio type III bursts observed by the Nançay
Radioheliograph from 1998 to 2008, covering nearly a full solar cycle. In particular, sources …
Radioheliograph from 1998 to 2008, covering nearly a full solar cycle. In particular, sources …
Formation and evolution of coherent structures in 3D strongly turbulent magnetized plasmas
We review the current literature on the formation of coherent structures (CoSs) in strongly
turbulent 3D magnetized plasmas. CoSs [Current Sheets (CS), magnetic filaments, large …
turbulent 3D magnetized plasmas. CoSs [Current Sheets (CS), magnetic filaments, large …
Statistical properties of magnetic activity in the solar corona
MK Georgoulis, M Velli, G Einaudi - The Astrophysical Journal, 1998 - iopscience.iop.org
The long-time statistical behavior of a two-dimensional section of a coronal loop subject to
random magnetic forcing is presented. The highly intermittent nature of dissipation is …
random magnetic forcing is presented. The highly intermittent nature of dissipation is …
Nanoflare statistics in an active region 3D MHD coronal model
Aims. We investigate the statistics for the spatial and temporal distribution of the energy input
into the corona in a three-dimensional magneto-hydrodynamical (3D MHD) model. The …
into the corona in a three-dimensional magneto-hydrodynamical (3D MHD) model. The …
Low-frequency radio observations of picoflare category energy releases in the solar atmosphere
We report low-frequency (80 MHz) radio observations of circularly polarized non-thermal
type I radio bursts (" noise storms") in the solar corona whose estimated energy is∼ 10 21 …
type I radio bursts (" noise storms") in the solar corona whose estimated energy is∼ 10 21 …